Infrared Properties Of AGB Stars: from Existing Databases to Antarctic Surveys
R. Guandalini, M. Busso
TL;DR
This paper reviews the infrared characteristics of AGB stars using existing data and discusses how future Antarctic surveys will enhance understanding of their late evolutionary stages, luminosities, and mass loss.
Contribution
It introduces the potential of Antarctic infrared surveys to improve quantitative knowledge of AGB stars' evolution, building on existing space-based data.
Findings
Preliminary analysis of C and S stars in infrared.
Future Antarctic surveys will be crucial for detailed studies.
Enhanced understanding of AGB star luminosities and mass loss.
Abstract
We present here a study of the Infrared properties of Asymptotic Giant Branch stars (hereafter AGB) based on existing databases, mainly from space-borne experiments. Preliminary results about C and S stars are discussed, focusing on the topics for which future Infrared surveys from Antarctica will be crucial. This kind of surveys will help in making more quantitative our knowledge of the last evolutionary stages of low mass stars, especially for what concerns luminosities and mass loss.
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